Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation | Paper Citation Record

Observation b611f8d1-d7bf-425a-9831-4eb14b0ddea4 · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.347120Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6f11f5b-8ccb-4f99-9f8d-e7bc90af8722 · outbound

This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.352201Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f2509c9-0dad-443b-97f9-09ee63bb53d8 · outbound

This paper cites The power spectrum and bispectrum of SDSS DR11 BOSS galaxies II: cosmological interpretation.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The power spectrum and bispectrum of SDSS DR11 BOSS galaxies II: cosmological interpretation

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.356950Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3b8445e-0519-43e5-a744-f58321411622 · outbound

This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.361440Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7bc47be-c50d-424f-a4e3-e1cc8e614003 · outbound

This paper cites The BOSS DR12 Full-Shape Cosmology: $\Lambda$CDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The BOSS DR12 Full-Shape Cosmology: $\Lambda$CDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.366005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 045084f1-f8f2-4b2f-bbb4-06b3d8e36b6a · outbound

This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.370486Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 32ade7dc-7610-42a1-a3d2-d54708c7adc9 · outbound

This paper cites {\sc SimBIG}: Cosmological Constraints using Simulation-Based Inference of Galaxy Clustering with Marked Power Spectra.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation {\sc SimBIG}: Cosmological Constraints using Simulation-Based Inference of Galaxy Clustering with Marked Power Spectra

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.375873Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f09f8c29-c556-47bb-9b7e-aa0ff7d2856b · outbound

This paper cites Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.380191Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b5b58cc3-6ccc-4240-8f9e-359276f7765f · outbound

This paper cites Cosmology behind the mask: Constraining the parameters of $\Lambda$CDM with the unmasked galaxy density field from VIPERS.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Cosmology behind the mask: Constraining the parameters of $\Lambda$CDM with the unmasked galaxy density field from VIPERS

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.384424Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95c0eb09-2897-43f4-8199-7b6777a361e8 · outbound

This paper cites A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.388553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f3bbada-3ad1-40d0-812f-1099b0f2bafc · outbound

This paper cites The VIMOS Public Extragalactic Redshift Survey (VIPERS): An unbiased estimate of the growth rate of structure at $\mathbf{\left<z\right>=0.85}$ using the clustering of luminous blue galaxies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The VIMOS Public Extragalactic Redshift Survey (VIPERS): An unbiased estimate of the growth rate of structure at $\mathbf{\left<z\right>=0.85}$ using the clustering of luminous blue galaxies

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.392673Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1abda63d-6b5b-438b-ac2a-67ae78c3eddb · outbound

This paper cites The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at $0.5<z<1.2$ from redshift-space distortions in the clustering of the PDR-2 final sample.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at $0.5<z<1.2$ from redshift-space distortions in the clustering of the PDR-2 final sample

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.396849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 21cddc33-8d1a-4641-8933-0c7c43774199 · outbound

This paper cites The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.403352Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7a78710c-c95d-4c5b-859a-fb0ea5d3d7db · outbound

This paper cites Information Content of the Angular Multipoles of Redshift-Space Galaxy Bispectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Information Content of the Angular Multipoles of Redshift-Space Galaxy Bispectrum

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.408919Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation baf2798d-99b9-489d-b83e-d6d1c224ca92 · outbound

This paper cites Full-Shape analysis of the power spectrum and bispectrum of DESI DR1 LRG and QSO samples.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Full-Shape analysis of the power spectrum and bispectrum of DESI DR1 LRG and QSO samples

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.413365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e070e88-c406-400e-bbba-548458f92ba2 · outbound

This paper cites The Redshift-Space Momentum Power Spectrum III: measuring the growth rate from the SDSSv survey using auto- and cross- power spectrum of the galaxy density and momentum fields.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The Redshift-Space Momentum Power Spectrum III: measuring the growth rate from the SDSSv survey using auto- and cross- power spectrum of the galaxy density and momentum fields

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.417579Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 77a04131-3a08-4e92-8941-0a45620f7a09 · outbound

This paper cites Brown, R.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Brown, R

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.421704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9b4e3b4b-6f46-44ae-a6d9-eadc7e93ac13 · outbound

This paper cites Limits on primordial non-Gaussianities from BOSS galaxy-clustering data.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Limits on primordial non-Gaussianities from BOSS galaxy-clustering data

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.425689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b91c6f35-aa6e-4478-bac5-83a6ae5eb5b8 · outbound

This paper cites Local primordial non-Gaussianity from the large-scale clustering of photometric DESI luminous red galaxies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Local primordial non-Gaussianity from the large-scale clustering of photometric DESI luminous red galaxies

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.430018Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8fb0f909-a882-49f0-96f6-0e7971dc041e · outbound

This paper cites Primordial non-Gaussianity, scale-dependent bias, and the bispectrum of galaxies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Primordial non-Gaussianity, scale-dependent bias, and the bispectrum of galaxies

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.434214Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bce549cc-80d3-4bba-aa44-f1943678292d · outbound

This paper cites The Clustering of Galaxies in SDSS-III DR9 Baryon Oscillation Spectroscopic Survey: Constraints on Primordial Non-Gaussianity.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The Clustering of Galaxies in SDSS-III DR9 Baryon Oscillation Spectroscopic Survey: Constraints on Primordial Non-Gaussianity

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.438422Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c4235e18-b78a-446b-9959-f846dee3595d · outbound

This paper cites an unresolved cited work.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Unresolved cited work

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.442605Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3e115aef-77ed-479d-8578-ee2e927d5037 · outbound

This paper cites Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.446598Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e363dc46-0666-4dd2-aa06-b85c3224c7f0 · outbound

This paper cites Galaxy redshift-space bispectrum: the Importance of Being Anisotropic.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Galaxy redshift-space bispectrum: the Importance of Being Anisotropic

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.450928Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 276db0b2-4214-4793-80f6-51bbe3298103 · outbound

This paper cites Squeezing $f_{\rm NL}$ out of the matter bispectrum with consistency relations.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Squeezing $f_{\rm NL}$ out of the matter bispectrum with consistency relations

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.455317Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 140a3399-4f95-4482-8987-5106cb9c1c38 · outbound

This paper cites GEO-FPT: a model of the galaxy bispectrum at mildly non-linear scales.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation GEO-FPT: a model of the galaxy bispectrum at mildly non-linear scales

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.459429Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 918ac6b7-06b8-40f6-b296-e67db9d73f3f · outbound

This paper cites Decoupling Local Primordial non-Gaussianity from Relativistic Effects in the Galaxy Bispectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Decoupling Local Primordial non-Gaussianity from Relativistic Effects in the Galaxy Bispectrum

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.463646Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4cf65871-38cb-4169-835c-47fa27565a59 · outbound

This paper cites A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - II: Fitting Techniques.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - II: Fitting Techniques

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.467795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation abeddddb-f3ab-4bf0-9080-db1a66453ae4 · outbound

This paper cites Detection of Baryon Acoustic Oscillation Features in the Large-Scale 3-Point Correlation Function of SDSS BOSS DR12 CMASS Galaxies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Detection of Baryon Acoustic Oscillation Features in the Large-Scale 3-Point Correlation Function of SDSS BOSS DR12 CMASS Galaxies

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.471881Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b3b966d2-97b9-4ce9-8b55-229c61d8c2bd · outbound

This paper cites A Detection of the Baryon Acoustic Oscillation Features in the SDSS BOSS DR12 Galaxy Bispectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation A Detection of the Baryon Acoustic Oscillation Features in the SDSS BOSS DR12 Galaxy Bispectrum

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.476036Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 44e04fea-3dbc-4656-8aa8-7a2b42e1bd1d · outbound

This paper cites Accelerating BAO Scale Fitting Using Taylor Series.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Accelerating BAO Scale Fitting Using Taylor Series

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.480463Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f701ba7-c1fd-46d2-9da4-f09a3ad1d3e9 · outbound

This paper cites Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.484583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f592269f-0360-44d9-ac8e-2ecb39dbbbdb · outbound

This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.488943Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 029f6705-f94b-4524-b546-ca01788c50c0 · outbound

This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.493164Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7662f22d-44fb-49c3-ac00-f4935ffd38b6 · outbound

This paper cites Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.497240Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2f728699-bad3-42e2-9175-5e5d4c607b5b · outbound

This paper cites First Detection of the BAO Signal from Early DESI Data.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation First Detection of the BAO Signal from Early DESI Data

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.501401Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e6fa5ae1-72b2-405e-80d4-3ba30648bc3c · outbound

This paper cites Modeling the BAO feature in Bispectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Modeling the BAO feature in Bispectrum

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.505534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d50888a-4f6c-4dc4-8986-deddfd156b39 · outbound

This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.509515Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 17d11bb2-fda6-4c7b-abca-5b135c0ccb4c · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.514023Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 345ad56f-5aad-4f2b-96e8-3f9c10cf8355 · outbound

This paper cites Constraining the Baryon-Dark Matter Relative Velocity with the Large-Scale 3-Point Correlation Function of the SDSS BOSS DR12 CMASS Galaxies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Constraining the Baryon-Dark Matter Relative Velocity with the Large-Scale 3-Point Correlation Function of the SDSS BOSS DR12 CMASS Galaxies

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.518359Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f60e8de-2cd8-4a22-b3c7-2e82509b5b7e · outbound

This paper cites The large-scale 3-point correlation function of the SDSS BOSS DR12 CMASS galaxies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The large-scale 3-point correlation function of the SDSS BOSS DR12 CMASS galaxies

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.522699Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cb558f61-1a78-4ef2-8164-95b078dd3223 · outbound

This paper cites On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.526690Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b2952dc-bb6f-49e1-8370-e8fd209a3e55 · outbound

This paper cites C$^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation C$^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.530989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 781b890f-ca2d-464f-89a4-4cd9ed526bb9 · outbound

This paper cites Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.535459Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 16134c2a-f9dd-42a6-930a-cc1af64321fd · outbound

This paper cites The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.539642Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aeca26e7-9201-4709-8a5b-a35422fef6a6 · outbound

This paper cites Bispectrum as Baryon Acoustic Oscillation Interferometer.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Bispectrum as Baryon Acoustic Oscillation Interferometer

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.543798Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ef2164d1-d0c8-448c-893e-03e666aa6fae · outbound

This paper cites Constraining galaxy-halo connection with high-order statistics.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Constraining galaxy-halo connection with high-order statistics

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.548086Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 810f98de-191c-40ff-8de5-334e5ab780dc · outbound

This paper cites Exploring the squeezed three-point galaxy correlation function with generalized halo occupation distribution models.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Exploring the squeezed three-point galaxy correlation function with generalized halo occupation distribution models

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.552420Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cbd83a0f-3f0f-4096-964a-3a39f7706687 · outbound

This paper cites Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.556528Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9cff87bd-f197-449b-b88d-beb611660614 · outbound

This paper cites Cosmological Three-Point Function: Testing The Halo Model Against Simulations.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Cosmological Three-Point Function: Testing The Halo Model Against Simulations

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.560758Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 19279a8b-5f16-410f-a5c2-1b5e5e8fb36c · outbound

This paper cites The DESI One-Percent survey: constructing galaxy-halo connections for ELGs and LRGs using auto and cross correlations.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The DESI One-Percent survey: constructing galaxy-halo connections for ELGs and LRGs using auto and cross correlations

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.565035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88357c51-5b63-4cfe-9d75-da7fa69639af · outbound

This paper cites Evidence for galaxy assembly bias in BOSS CMASS redshift-space galaxy correlation function.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Evidence for galaxy assembly bias in BOSS CMASS redshift-space galaxy correlation function

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.569426Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b235751-cce1-4213-86c6-413af4bdc320 · outbound

This paper cites Extensions to models of the galaxy-halo connection.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Extensions to models of the galaxy-halo connection

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.573747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bed23c3f-38fd-4325-91a7-da0b61b6b8fb · outbound

This paper cites How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.578178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4f7cfe44-f39d-46cb-b344-4173d4131a85 · outbound

This paper cites Information content in the halo-model dark-matter power spectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Information content in the halo-model dark-matter power spectrum

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.582623Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a56ff5ab-e901-4fb5-bb3b-c06ec72f85ef · outbound

This paper cites Information content in the halo-model dark-matter power spectrum II: Multiple cosmological parameters.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Information content in the halo-model dark-matter power spectrum II: Multiple cosmological parameters

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.586926Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fc3fcee4-3f80-4ad6-a8cb-7c91cff5755c · outbound

This paper cites Redshift-Space Clustering of SDSS Galaxies --- Luminosity Dependence, Halo Occupation Distribution, and Velocity Bias.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Redshift-Space Clustering of SDSS Galaxies --- Luminosity Dependence, Halo Occupation Distribution, and Velocity Bias

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.591246Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d95ddedb-e67a-4bc1-abdf-9f9495d8c31f · outbound

This paper cites The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.595482Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3bf67f17-b3d1-4fea-9348-9bd21fea3419 · outbound

This paper cites Construct the emission line galaxy-host halo connection through auto and cross correlations.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Construct the emission line galaxy-host halo connection through auto and cross correlations

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.599594Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 16980efa-1db6-4e18-b8fc-21732288b4c7 · outbound

This paper cites The Power Spectrum Dependence of Dark Matter Halo Concentrations.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The Power Spectrum Dependence of Dark Matter Halo Concentrations

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.603776Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2704be7d-fc97-4389-893d-d0dedaa18fae · outbound

This paper cites Neutrino Mass Signatures in the Galaxy Bispectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Neutrino Mass Signatures in the Galaxy Bispectrum

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.607845Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 07c9695f-f4ac-46f5-9ac2-fa6ae575e490 · outbound

This paper cites Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.612019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d7ad3ada-290a-4322-b284-df5737b8b45a · outbound

This paper cites Neutrino footprint in Large Scale Structure.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Neutrino footprint in Large Scale Structure

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.616347Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0bc61409-0dc6-4256-b03e-0ccd664b5581 · outbound

This paper cites Neutrino mass limits: robust information from the power spectrum of galaxy surveys.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Neutrino mass limits: robust information from the power spectrum of galaxy surveys

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.620795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df7e77e0-95b4-456f-97ee-a59595712f2a · outbound

This paper cites Constraining $M_\nu$ with the Bispectrum I: Breaking Parameter Degeneracies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Constraining $M_\nu$ with the Bispectrum I: Breaking Parameter Degeneracies

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.625053Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e0b3962-632c-4369-a5a9-896457efec0d · outbound

This paper cites Constraining $M_\nu$ with the Bispectrum II: The Total Information Content of the Galaxy Bispectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Constraining $M_\nu$ with the Bispectrum II: The Total Information Content of the Galaxy Bispectrum

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.629298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7967138d-7e0e-451b-a72f-0629530cf132 · outbound

This paper cites DEMNUni: Massive neutrinos and the bispectrum of large scale structures.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation DEMNUni: Massive neutrinos and the bispectrum of large scale structures

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.634089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0588b51f-716e-44e1-a198-b778ed0b0918 · outbound

This paper cites Tree-Level Bispectrum in the Effective Field Theory of Large-Scale Structure extended to Massive Neutrinos.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Tree-Level Bispectrum in the Effective Field Theory of Large-Scale Structure extended to Massive Neutrinos

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.638417Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f192dc79-8d97-42ef-863d-87d1ed74e587 · outbound

This paper cites Developing the 3-Point Correlation Function For the Turbulent Interstellar Medium.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Developing the 3-Point Correlation Function For the Turbulent Interstellar Medium

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.642849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0edf8150-dc10-4ada-bedb-ef6f8302ab26 · outbound

This paper cites Studying Interstellar Turbulence Driving Scales using the Bispectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Studying Interstellar Turbulence Driving Scales using the Bispectrum

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.646919Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 24a702bb-db75-4140-b53f-856f1dae3af7 · outbound

This paper cites Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.651753Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e2b22802-ba89-4673-a1dd-44dfd9cd4fec · outbound

This paper cites First Measurements of the 4-Point Correlation Function of Magnetohydrodynamic Turbulence as a Novel Probe of the Interstellar Medium.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation First Measurements of the 4-Point Correlation Function of Magnetohydrodynamic Turbulence as a Novel Probe of the Interstellar Medium

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.655923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4794702e-0ab5-4b82-aee4-916978643faa · outbound

This paper cites Non-Gaussianity from Inflation: Theory and Observations.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Non-Gaussianity from Inflation: Theory and Observations

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.660093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 04492fc1-ee40-4d09-a12f-6b49892592ba · outbound

This paper cites A First Detection of the Connected 4-Point Correlation Function of Galaxies Using the BOSS CMASS Sample.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation A First Detection of the Connected 4-Point Correlation Function of Galaxies Using the BOSS CMASS Sample

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.664340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 185500bd-5a57-4f33-a7d3-34137ac5a261 · outbound

This paper cites Accelerating the 2-point and 3-point galaxy correlation functions using Fourier transforms.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Accelerating the 2-point and 3-point galaxy correlation functions using Fourier transforms

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.668737Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a73d0621-b99f-4497-bb9a-7bf3f704a603 · outbound

This paper cites A new look at lines of sight: using Fourier methods for the wide-angle anisotropic 2-point correlation function.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation A new look at lines of sight: using Fourier methods for the wide-angle anisotropic 2-point correlation function

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.673146Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39e343de-84a2-465d-88e5-29396136a486 · outbound

This paper cites SARABANDE: 3/4 Point Correlation Functions with Fast Fourier Transforms.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation SARABANDE: 3/4 Point Correlation Functions with Fast Fourier Transforms

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.677505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6dbfba4e-6d6c-40a2-b2a8-7a0bc1f4c654 · outbound

This paper cites Efficient Computation of $N$-point Correlation Functions in $D$ Dimensions.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Efficient Computation of $N$-point Correlation Functions in $D$ Dimensions

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.681906Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f38a73e-cd08-4f2f-98f3-3f054bfc48a2 · outbound

This paper cites Brown, G.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Brown, G

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.686401Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e45a8cc-4c7c-4ea8-baf0-1ded5f039e0e · outbound

This paper cites 2-FAST: Fast and accurate computation of projected two-point functions.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation 2-FAST: Fast and accurate computation of projected two-point functions

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.690439Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 15b18dd8-6a63-403b-ba60-61b354a391f2 · outbound

This paper cites Modelling the next-to-leading order matter three-point correlation function using FFTLog.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Modelling the next-to-leading order matter three-point correlation function using FFTLog

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.694624Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a50b8657-e046-4562-b445-3416a4be2458 · outbound

This paper cites PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation PolyBin3D: A Suite of Optimal and Efficient Power Spectrum and Bispectrum Estimators for Large-Scale Structure

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.698681Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b87415e1-d109-4e73-9c72-53c042eedef5 · outbound

This paper cites Cosmological Angular Trispectra and Non-Gaussian Covariance.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Cosmological Angular Trispectra and Non-Gaussian Covariance

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.702978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 81c5fa36-1f0c-44ba-8b20-49878ba09473 · outbound

This paper cites The Galaxy Bispectrum in the Spherical Fourier-Bessel Basis.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The Galaxy Bispectrum in the Spherical Fourier-Bessel Basis

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.707305Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f6ea0ca8-57a4-44df-a96e-8b8ab4111328 · outbound

This paper cites Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Exact Modeling of Power Spectrum Multipole through Spherical Fourier-Bessel Basis

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.711412Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 55444f45-995a-4a1e-9494-a962edf18a0c · outbound

This paper cites Fast Theoretical Predictions for Spherical Fourier Analysis of Large-Scale Structures.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Fast Theoretical Predictions for Spherical Fourier Analysis of Large-Scale Structures

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.715641Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c5c992ad-dbe1-4e80-9e33-16764341bcec · outbound

This paper cites Validation of Spherical Fourier-Bessel power spectrum analysis with lognormal simulations and eBOSS DR16 LRG EZmocks.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Validation of Spherical Fourier-Bessel power spectrum analysis with lognormal simulations and eBOSS DR16 LRG EZmocks

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.719927Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa0657e3-5f42-4434-863f-35deb567e311 · outbound

This paper cites The full-sky Spherical Fourier-Bessel power spectrum in general relativity.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation The full-sky Spherical Fourier-Bessel power spectrum in general relativity

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.724165Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 179274fd-0468-496f-9481-250243640ac6 · outbound

This paper cites Graph Database Solution for Higher Order Spatial Statistics in the Era of Big Data.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Graph Database Solution for Higher Order Spatial Statistics in the Era of Big Data

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.728426Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 87dca5e2-404e-4ba9-a116-44343fc1e0fe · outbound

This paper cites Gramsci: GRAph Made Statistics for Cosmological Information.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Gramsci: GRAph Made Statistics for Cosmological Information

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.732709Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6613997d-4cd5-482e-aaba-5a0f48eecf17 · outbound

This paper cites Demina, S.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Demina, S

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.736839Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 74569299-2b61-4a10-a9e6-448a073327e4 · outbound

This paper cites Computing the Small-Scale Galaxy Power Spectrum and Bispectrum in Configuration-Space.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Computing the Small-Scale Galaxy Power Spectrum and Bispectrum in Configuration-Space

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.740808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0a64a1b2-f1f7-4fcb-9224-096c110f665e · outbound

This paper cites A Faster Fourier Transform? Computing Small-Scale Power Spectra and Bispectra for Cosmological Simulations in $\mathcal{O}(N^2)$ Time.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation A Faster Fourier Transform? Computing Small-Scale Power Spectra and Bispectra for Cosmological Simulations in $\mathcal{O}(N^2)$ Time

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.745105Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 884c7e04-0a74-48fd-90ca-7468bd69d00e · outbound

This paper cites Neural Network-based model of galaxy power spectrum: Fast full-shape galaxy power spectrum analysis.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Neural Network-based model of galaxy power spectrum: Fast full-shape galaxy power spectrum analysis

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.749384Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8eeb8078-7657-4ecb-90c3-882d10f6d019 · outbound

This paper cites FREmu: Power Spectrum Emulator for $f(R)$ Gravity.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation FREmu: Power Spectrum Emulator for $f(R)$ Gravity

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.753850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b1f106ff-5ea7-4063-865d-9830760e07ea · outbound

This paper cites $\texttt{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation $\texttt{matryoshka}$: Halo Model Emulator for the Galaxy Power Spectrum

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.758026Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e55f093-99f9-43f0-b443-e6c38b1cf771 · outbound

This paper cites $\texttt{matryoshka}$ II: Accelerating Effective Field Theory Analyses of the Galaxy Power Spectrum.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation $\texttt{matryoshka}$ II: Accelerating Effective Field Theory Analyses of the Galaxy Power Spectrum

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.762251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 00210599-c842-4f8f-9293-af5d27912dfb · outbound

This paper cites PkANN - I. Non-linear matter power spectrum interpolation through artificial neural networks.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation PkANN - I. Non-linear matter power spectrum interpolation through artificial neural networks

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.766305Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bf81093b-f3de-4976-8a09-3da1d952bdca · outbound

This paper cites PkANN - II. A non-linear matter power spectrum interpolator developed using artificial neural networks.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation PkANN - II. A non-linear matter power spectrum interpolator developed using artificial neural networks

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.770589Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e85113b0-3cae-4184-90cd-231d2f733e7a · outbound

This paper cites Computing the Three-Point Correlation Function of Galaxies in $\mathcal{O}(N^2)$ Time.

Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation Computing the Three-Point Correlation Function of Galaxies in $\mathcal{O}(N^2)$ Time

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-16T05:21:13.774575Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Coverage vector

Reference resolution

Outbound references

Pith citing papers